Search Publications

Statistical evidence for O+ energization and outflow caused by wave-particle interaction in the high altitude cusp and mantle
DOI: 10.5194/angeo-29-945-2011 Bibcode: 2011AnGeo..29..945W

Waara, M.; Nilsson, H.; Slapak, R. +3 more

We present a statistical study of the low (<1 Hz) frequency electric and magnetic field spectral densities observed by Cluster spacecraft in the high altitude cusp and mantle region. At the O+ gyrofrequency (0.02-0.5 Hz) for this region the electric field spectral density is on average 0.2-2.2 (mV m-1)2 Hz-…

2011 Annales Geophysicae
Cluster 28
Cluster observations of trapped ions interacting with magnetosheath mirror modes
DOI: 10.5194/angeo-29-1049-2011 Bibcode: 2011AnGeo..29.1049S

Escoubet, C. P.; Soucek, J.

Mirror modes are among the most intense low frequency plasma wave phenomena observed in the magnetosheaths of magnetized planets. They appear as large amplitude non-propagating fluctuations in the magnetic field magnitude and plasma density. These structures are widely accepted to represent a non-linear stage of the mirror instability, dominant in…

2011 Annales Geophysicae
Cluster 28
The distribution of the ring current: Cluster observations
DOI: 10.5194/angeo-29-1655-2011 Bibcode: 2011AnGeo..29.1655Z

Woodfield, E. E.; Lockwood, M.; Dunlop, M. W. +9 more

Extending previous studies, a full-circle investigation of the ring current has been made using Cluster 4-spacecraft observations near perigee, at times when the Cluster array had relatively small separations and nearly regular tetrahedral configurations, and when the Dst index was greater than -30 nT (non-storm conditions). These observations res…

2011 Annales Geophysicae
Cluster 27
Accuracy of multi-point boundary crossing time analysis
DOI: 10.5194/angeo-29-2239-2011 Bibcode: 2011AnGeo..29.2239V

Haaland, S.; Paschmann, G.; Vogt, J.

Recent multi-spacecraft studies of solar wind discontinuity crossings using the timing (boundary plane triangulation) method gave boundary parameter estimates that are significantly different from those of the well-established single-spacecraft minimum variance analysis (MVA) technique. A large survey of directional discontinuities in Cluster data…

2011 Annales Geophysicae
Cluster 23
Comparison of accelerated ion populations observed upstream of the bow shocks at Venus and Mars
DOI: 10.5194/angeo-29-511-2011 Bibcode: 2011AnGeo..29..511Y

Coates, A. J.; Fedorov, A.; Barabash, S. +12 more

Foreshock ions are compared between Venus and Mars at energies of 0.6~20 keV using the same ion instrument, the Ion Mass Analyser, on board both Venus Express and Mars Express. Venus Express often observes accelerated protons (2~6 times the solar wind energy) that travel away from the Venus bow shock when the spacecraft location is magnetically co…

2011 Annales Geophysicae
MEx VenusExpress 22
Non-stationarity of the quasi-perpendicular bow shock: comparison between Cluster observations and simulations
DOI: 10.5194/angeo-29-263-2011 Bibcode: 2011AnGeo..29..263C

Scholer, M.; Soucek, J.; Comişel, H. +1 more

We have performed full particle electromagnetic simulations of a quasi-perpendicular shock. The shock parameters have been chosen to be appropriate for the quasi-perpendicular Earth's bow shock observed by Cluster on 24 January 2001 (Lobzin et al., 2007). We have performed two simulations with different ion to electron mass ratio: run 1 with m

2011 Annales Geophysicae
Cluster 22
O+ heating associated with strong wave activity in the high altitude cusp and mantle
DOI: 10.5194/angeo-29-931-2011 Bibcode: 2011AnGeo..29..931S

Waara, M.; Nilsson, H.; Slapak, R. +3 more

We use the Cluster spacecraft to study three events with intense waves and energetic oxygen ions (O+) in the high altitude cusp and mantle. The ion energies considered are of the order 1000 eV and higher, observed above an altitude of 8 earth radii together with high wave power at the O+ gyrofrequency. We show that heating by…

2011 Annales Geophysicae
Cluster 22
Magnetospheric mapping of the dayside UV auroral oval at Saturn using simultaneous HST images, Cassini IMF data, and a global magnetic field model
DOI: 10.5194/angeo-29-1233-2011 Bibcode: 2011AnGeo..29.1233B

Belenkaya, E. S.; Nichols, J. D.; Cowley, S. W. H. +2 more

We determine the field-aligned mapping of Saturn's auroras into the magnetosphere by combining UV images of the southern dayside oval obtained by the Hubble Space Telescope (HST) with a global model of the magnetospheric magnetic field. The model is tailored to simulate prevailing conditions in the interplanetary medium, corresponding to high sola…

2011 Annales Geophysicae
Cassini eHST 20
Analysis of ionospheric electrodynamic parameters on mesoscales - a review of selected techniques using data from ground-based observation networks and satellites
DOI: 10.5194/angeo-29-467-2011 Bibcode: 2011AnGeo..29..467V

Amm, O.; Vanhamäki, H.

We present a review of selected data-analysis methods that are frequently applied in studies of ionospheric electrodynamics and magnetosphere-ionosphere coupling using ground-based and space-based data sets. Our focus is on methods that are data driven (not simulations or statistical models) and can be used in mesoscale studies, where the analysis…

2011 Annales Geophysicae
Cluster 20
The statistical studies of the inner boundary of plasma sheet
DOI: 10.5194/angeo-29-289-2011 Bibcode: 2011AnGeo..29..289C

Dandouras, I.; Cao, J. B.; Ding, W. Z. +4 more

The penetration of plasma sheet ions into the inner magnetosphere is very important to the inner magnetospheric dynamics since plasma sheet ions are one of the major particle sources of ring current during storm times. However, the direct observations of the inner boundary of the plasma sheet are fairly rare due to the limited number of satellites…

2011 Annales Geophysicae
DoubleStar 19